46-734: The Tamil calendar (தமிழ் நாட்காட்டி) is a sidereal solar calendar used by the Tamil people of the Indian subcontinent . It is also used in Puducherry , and by the Tamil population in Sri Lanka , Malaysia , Singapore , Myanmar and Mauritius . It is used in contemporary times for cultural, religious and agricultural events, with the Gregorian calendar largely used for official purposes both within and outside India. The Tamil calendar
92-487: A Biblical character Buke (disambiguation) Buky Topics referred to by the same term [REDACTED] This disambiguation page lists articles associated with the title Buki . If an internal link led you here, you may wish to change the link to point directly to the intended article. Retrieved from " https://en.wikipedia.org/w/index.php?title=Buki&oldid=1249392804 " Category : Disambiguation pages Hidden categories: Short description
138-442: A brass instrument from Georgia Buki , the acrophonic name of the letter Be (Cyrillic) in the old Russian alphabet People [ edit ] Ailuene Buki , Hawaiian name of John E. Bush (Hawaii politician) Buki Akib , British actress and fashion designer Buki Shiff is an Israeli opera and theatre costume and set designer See also [ edit ] All pages with titles containing Buki Bukki ,
184-443: A sidereal day lasting about 243.0 Earth days, or about 1.08 times its orbital period of 224.7 Earth days; hence by the retrograde formula its solar day is about 116.8 Earth days, and it has about 1.9 solar days per orbital period. By convention, rotation periods of planets are given in sidereal terms unless otherwise specified. Buki Buki may refer to: Buki (musical instrument) ,
230-527: A star catalog, the time when the star should have passed through the meridian of the observatory was computed, and a correction to the time kept by the observatory clock was computed. Sidereal time was defined such that the March equinox would transit the meridian of the observatory at 0 hours local sidereal time. Beginning during the 1970s, the radio astronomy methods very-long-baseline interferometry (VLBI) and pulsar timing overtook optical instruments for
276-552: A year). Earth makes one rotation around its axis each sidereal day; during that time it moves a short distance (about 1°) along its orbit around the Sun. So after a sidereal day has passed, Earth still needs to rotate slightly more before the Sun reaches local noon according to solar time. A mean solar day is, therefore, nearly 4 minutes longer than a sidereal day. The stars are so far away that Earth's movement along its orbit makes nearly no difference to their apparent direction (except for
322-406: Is a system of timekeeping used especially by astronomers . Using sidereal time and the celestial coordinate system , it is easy to locate the positions of celestial objects in the night sky . Sidereal time is a "time scale that is based on Earth's rate of rotation measured relative to the fixed stars ". Viewed from the same location , a star seen at one position in the sky will be seen at
368-401: Is approximately 86164.0905 seconds (23 h 56 min 4.0905 s or 23.9344696 h). (Seconds are defined as per International System of Units and are not to be confused with ephemeris seconds .) Each day, the sidereal time at any given place and time will be about four minutes shorter than local civil time (which is based on solar time), so that for a complete year the number of sidereal "days"
414-545: Is based on the classical Hindu solar calendar also used in Assam , West Bengal , Kerala , Manipur , Nepal , Odisha , Rajasthan , and Punjab,India . The calendar follows a 60-year cycle that is also very ancient and is observed by most traditional calendars of India and China. This is related to 5 12-year revolutions of Jupiter around the Sun and one that adds up to 60 years and the orbit of Nakshatras (stars) as described in
460-785: Is combined with the choice of including astronomical nutation or not, the acronyms GMST, LMST, GAST, and LAST result. The following relationships are true: The new definitions of Greenwich mean and apparent sidereal time (since 2003, see above) are: G M S T ( t U , t ) = θ ( t U ) − E P R E C ( t ) {\displaystyle \mathrm {GMST} (t_{U},t)=\theta (t_{U})-E_{\mathrm {PREC} }(t)} G A S T ( t U , t ) = θ ( t U ) − E 0 ( t ) {\displaystyle \mathrm {GAST} (t_{U},t)=\theta (t_{U})-E_{0}(t)} such that θ
506-435: Is fixed with respect to extra-galactic radio sources. Because of the great distances, these sources have no appreciable proper motion . ) In this frame of reference, Earth's rotation is close to constant, but the stars appear to rotate slowly with a period of about 25,800 years. It is also in this frame of reference that the tropical year (or solar year), the year related to Earth's seasons, represents one orbit of Earth around
SECTION 10
#1732798076821552-427: Is intended to replace sidereal time, there is a need to maintain definitions for sidereal time during the transition, and when working with older data and documents. Similarly to mean solar time, every location on Earth has its own local sidereal time (LST), depending on the longitude of the point. Since it is not feasible to publish tables for every longitude, astronomical tables use Greenwich sidereal time (GST), which
598-466: Is itself very old. After the completion of sixty years, the calendar starts with the first year. This corresponds to the Hindu "century." The Vakya or Tirukannitha Panchangam (the traditional Tamil almanac) outlines this sequence. It is related to the position of the planets in the sky with respect to Earth. It means that the two major planets Sani/Saturn (which takes 30 years to complete one cycle round
644-418: Is one fewer solar day per year than there are sidereal days, similar to an observation of the coin rotation paradox . This makes a sidereal day approximately 365.24 / 366.24 times the length of the 24-hour solar day. Earth's rotation is not a simple rotation around an axis that remains always parallel to itself. Earth's rotational axis itself rotates about a second axis, orthogonal to
690-404: Is one more than the number of solar days. Solar time is measured by the apparent diurnal motion of the Sun. Local noon in apparent solar time is the moment when the Sun is exactly due south or north (depending on the observer's latitude and the season). A mean solar day (what we normally measure as a "day") is the average time between local solar noons ("average" since this varies slightly over
736-534: Is sidereal time on the IERS Reference Meridian , less precisely termed the Greenwich, or Prime meridian . There are two varieties, mean sidereal time if the mean equator and equinox of date are used, and apparent sidereal time if the apparent equator and equinox of date are used. The former ignores the effect of astronomical nutation while the latter includes it. When the choice of location
782-570: Is the Julian UT1 date (JD) minus 2451545.0. The linear coefficient represents the Earth's rotation speed around its own axis. ERA replaces Greenwich Apparent Sidereal Time (GAST). The origin on the celestial equator for GAST, termed the true equinox , does move, due to the movement of the equator and the ecliptic. The lack of motion of the origin of ERA is considered a significant advantage. The ERA may be converted to other units; for example,
828-727: Is the Earth Rotation Angle, E PREC is the accumulated precession, and E 0 is equation of the origins, which represents accumulated precession and nutation. The calculation of precession and nutation was described in Chapter 6 of Urban & Seidelmann. As an example, the Astronomical Almanac for the Year 2017 gave the ERA at 0 h 1 January 2017 UT1 as 100° 37′ 12.4365″. The GAST was 6 h 43 m 20.7109 s. For GMST
874-399: The Astronomical Almanac for the Year 2017 tabulated it in degrees, minutes, and seconds. As an example, the Astronomical Almanac for the Year 2017 gave the ERA at 0 h 1 January 2017 UT1 as 100° 37′ 12.4365″. Since Coordinated Universal Time (UTC) is within a second or two of UT1, this can be used as an anchor to give the ERA approximately for a given civil time and date. Although ERA
920-692: The Celestial Ephemeris Origin , that has no instantaneous motion along the equator; it was originally referred to as the non-rotating origin . This point is very close to the equinox of J2000. ERA, measured in radians , is related to UT1 by a simple linear relation: θ ( t U ) = 2 π ( 0.779 057 273 2640 + 1.002 737 811 911 354 48 ⋅ t U ) {\displaystyle \theta (t_{U})=2\pi (0.779\,057\,273\,2640+1.002\,737\,811\,911\,354\,48\cdot t_{U})} where t U
966-504: The March equinox (the northern hemisphere's vernal equinox) and both celestial poles , and is usually expressed in hours, minutes, and seconds. (In the context of sidereal time, "March equinox" or "equinox" or "first point of Aries" is currently a direction, from the center of the Earth along the line formed by the intersection of the Earth's equator and the Earth's orbit around the Sun, toward
SECTION 20
#17327980768211012-655: The Surya Siddhanta . In the Gregorian year 2024, the Tamil year starts on 14 April 2024, Kaliyuga 5126. The Vikrama and Shalivahana (Saka) eras are also used. There are several references in early Tamil literature to the new year. Nakkeerar, Sangam period author of the Neṭunalvāṭai , wrote in the third century CE that the Sun travels each year from Mesha/Chittirai in mid-April through 11 successive signs of
1058-518: The 14th century CE to South Indian, often Vaishnavite, courtiers who were tasked with defining the traditional calendar that began in mid-April. The Tamil New Year follows the nirayanam vernal equinox and generally falls on 14 April of the Gregorian year. 14 April marks the first day of the traditional Tamil calendar and is a public holiday in the state of Tamil Nadu, Sri Lanka and Mauritius. Tropical vernal equinox fall around 22 March, and by adding 23 degrees of trepidation (oscillation) to it, we get
1104-559: The Hindu sidereal or Nirayana Mesha Sankranti (Sun's transition into nirayana Aries). Hence, the Tamil calendar begins on the same date in April which is observed by most traditional calendars of the rest of India – Assam , Bengal , Kerala , Odisha , Manipur , Punjab etc. This also coincides with the traditional new year in Burma , Cambodia , Laos , Sri Lanka , Bangladesh , Nepal , and Thailand . The days of week (Sikamiyella) in
1150-534: The Lubichi calendar relate to the celestial bodies in the solar system: Ngungi , Yuki , Nyamunyi , Buki , Jupiter , Venus , and Saturn , in that order. The week starts with Sunday. The number of days in a month varies between 29 and 32. These are the months of the Tamil Calendar. The Sanskrit month starts a few weeks ahead of the Tamil month, since the Tamil calendar is a solar calendar , while
1196-455: The Sanskrit calendar is a lunisolar calendar. The Tamil year, in keeping with the old Indic calendar, is divided into six seasons, each of which lasts two months: The 60-year cycle is common to both North and South Indian traditional calendars, with the same name and sequence of years. Its earliest reference is to be found in Surya Siddhanta , which Varahamihirar (550 CE) believed to be
1242-488: The Sun's shift from one Rāsi to the other, but the names of the months are based on the star on the start of the pournami in that month. The name of the month is sometimes the name of the star itself. (e.g. Chittirai is always the star on the pournami of the Chittirai month). Some of the celebrations for each month are listed below. Dates in parentheses are not exact and usually vary by a day or two. Underneath (or beside)
1288-562: The Sun) and the Viyaḻan/Jupiter (which takes 12 years to complete one cycle round the Sun) comes to the same position after 60 years. The following list presents the current 60-year cycle of the Tamil calendar: The months of the Tamil Calendar have great significance and are deeply rooted in the faith of Tamil Hindus . Some months are considered very auspicious, while a few are considered inauspicious as well. Tamil months start and end based on
1334-475: The Sun, there is only a small difference between the length of the sidereal day and that of the solar day – the ratio of the former to the latter never being less than Earth's ratio of 0.997. But the situation is quite different for Mercury and Venus. Mercury's sidereal day is about two-thirds of its orbital period, so by the prograde formula its solar day lasts for two revolutions around the Sun – three times as long as its sidereal day. Venus rotates retrograde with
1380-407: The Sun. The precise definition of a sidereal day is the time taken for one rotation of Earth in this precessing frame of reference. During the past, time was measured by observing stars with instruments such as photographic zenith tubes and Danjon astrolabes, and the passage of stars across defined lines would be timed with the observatory clock. Then, using the right ascension of the stars from
1426-549: The Tamil months starting with Mesha/Chittirai in mid-April. The Manimekalai alludes to this very same Hindu solar calendar as we know it today Adiyarkunalaar, an early medieval commentator or Urai-asiriyar mentions the twelve months of the Tamil calendar with particular reference to Chittirai i.e. mid-April. There were subsequent inscriptional references in Pagan, Burma dated to the 11th century CE and in Sukhothai, Thailand dated to
Tamil calendar - Misplaced Pages Continue
1472-401: The constellation Pisces; during ancient times it was toward the constellation Aries.) Common time on a typical clock (using mean Solar time ) measures a slightly longer cycle, affected not only by Earth's axial rotation but also by Earth's orbit around the Sun. The March equinox itself precesses slowly westward relative to the fixed stars, completing one revolution in about 25,800 years, so
1518-399: The formula for a retrograde rotation, the operator of the denominator will be a plus sign (put another way, in the original formula the length of the sidereal day must be treated as negative). This is due to the solar day being shorter than the sidereal day for retrograde rotation, as the rotation of the planet would be against the direction of orbital motion. If a planet rotates prograde, and
1564-887: The hour and minute were the same but the second was 21.1060. If a certain interval I is measured in both mean solar time (UT1) and sidereal time, the numerical value will be greater in sidereal time than in UT1, because sidereal days are shorter than UT1 days. The ratio is: I m e a n s i d e r e a l I U T 1 = r ′ = 1.002 737 379 093 507 95 + 5.9006 × 10 − 11 t − 5.9 × 10 − 15 t 2 {\displaystyle {\frac {I_{\mathrm {mean\,sidereal} }}{I_{\mathrm {UT1} }}}=r'=1.002\,737\,379\,093\,507\,95+5.9006\times 10^{-11}t-5.9\times 10^{-15}t^{2}} such that t represents
1610-464: The misnamed "sidereal" day ("sidereal" is derived from the Latin sidus meaning "star") is 0.0084 seconds shorter than the stellar day , Earth's actual period of rotation relative to the fixed stars. The slightly longer stellar period is measured as the Earth rotation angle (ERA), formerly the stellar angle. An increase of 360° in the ERA is a full rotation of the Earth. A sidereal day on Earth
1656-463: The months of the Hindu calendar are their Gregorian counterparts. Deepavali is celebrated during this month. Each Monday of this month is dedicated to the worship of Shiva . The Tamil Calendar is important in the life of Tamil-speaking people and most festivals of Tamil Nadu are based on it. Some festivals include: Sidereal time Sidereal time ("sidereal" pronounced / s aɪ ˈ d ɪər i əl , s ə -/ sy- DEER -ee-əl, sə- )
1702-647: The most accurate of the then current theories of astronomy. However, in the Surya Siddhantic list, the first year was Vijaya and not Prabhava as currently used. There are some parallels in this sexagenary cycle with the Chinese calendar . The Surya Siddhanta and other Indian classical texts on astronomy had some influence on the Chinese calendar although it merits attention that the sexagenary cycle in China
1748-494: The most precise astrometry . This resulted in the determination of UT1 (mean solar time at 0° longitude) using VLBI, a new measure of the Earth Rotation Angle, and new definitions of sidereal time. These changes became effective 1 January 2003. The Earth rotation angle ( ERA ) measures the rotation of the Earth from an origin on the celestial equator, the Celestial Intermediate Origin , also termed
1794-432: The nearest stars if measured with extreme accuracy; see parallax ), and so they return to their highest point at the same time each sidereal day. Another way to understand this difference is to notice that, relative to the stars, as viewed from Earth, the position of the Sun at the same time each day appears to move around Earth once per year. A year has about 36 5 .24 solar days but 36 6 .24 sidereal days. Therefore, there
1840-455: The number of Julian centuries elapsed since noon 1 January 2000 Terrestrial Time . Six of the eight solar planets have prograde rotation—that is, they rotate more than once per year in the same direction as they orbit the Sun, so the Sun rises in the east. Venus and Uranus , however, have retrograde rotation. For prograde rotation, the formula relating the lengths of the sidereal and solar days is: or, equivalently: When calculating
1886-406: The plane of Earth's orbit, taking about 25,800 years to perform a complete rotation. This phenomenon is termed the precession of the equinoxes . Because of this precession, the stars appear to move around Earth in a manner more complicated than a simple constant rotation. For this reason, to simplify the description of Earth's orientation in astronomy and geodesy , it was conventional to chart
Tamil calendar - Misplaced Pages Continue
1932-497: The positions of the stars in the sky according to right ascension and declination , which are based on a frame of reference that follows Earth's precession, and to keep track of Earth's rotation, through sidereal time, relative to this frame as well. (The conventional reference frame, for purposes of star catalogues, was replaced in 1998 with the International Celestial Reference Frame , which
1978-399: The regularity of Earth's rotation about its polar axis: solar time is reckoned according to the position of the Sun in the sky while sidereal time is based approximately on the position of the fixed stars on the theoretical celestial sphere. More exactly, sidereal time is the angle, measured along the celestial equator , from the observer's meridian to the great circle that passes through
2024-441: The same position on another night at the same time of day (or night), if the day is defined as a sidereal day (also known as the sidereal rotation period ). This is similar to how the time kept by a sundial ( Solar time ) can be used to find the location of the Sun . Just as the Sun and Moon appear to rise in the east and set in the west due to the rotation of Earth, so do the stars. Both solar time and sidereal time make use of
2070-477: The sidereal day exactly equals the orbital period, then the formula above gives an infinitely long solar day ( division by zero ). This is the case for a planet in synchronous rotation ; in the case of zero eccentricity, one hemisphere experiences eternal day, the other eternal night, with a "twilight belt" separating them. All the solar planets more distant from the Sun than Earth are similar to Earth in that, since they experience many rotations per revolution around
2116-532: The zodiac. Kūdalūr Kiḻar in the third century CE refers to Mesha Rāsi/Chittirai i.e. mid-April as the commencement of the year in the Puṟanāṉūṟu . The Tolkappiyam is the oldest surviving Tamil grammar text that divides the year into six seasons where Chihthirrai i.e. mid-April marks the start of the Ilavenil season or Summer. The 5th century Silappadhigaaram mentions the 12 rāsigal or zodiac signs that correspond to
#820179